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About

Yuki Sarugaku is an observational astrophysicist whose work bridges instrumental innovation and high-energy astrophysics. A key figure in wide-field optical astronomy, Sarugaku led the development of the Kiso Wide Field Camera (KWFC), a four-square-degree facility instrument for the Kiso Schmidt Telescope. This camera, detailed in a 2012 paper with 39 citations, harnesses eight CCDs to exploit the telescope’s large focal plane, enabling transformative surveys of transient phenomena and galactic structures. Sarugaku’s impact extends to gamma-ray burst (GRB) physics, notably through early-time broadband modeling of GRB 051111 (2006, 38 citations). By integrating contemporaneous KAIT robotic telescope imaging with multi-wavelength data, this work probed the critical transition between internal and external shocks—a cornerstone question in GRB afterglow theory. These contributions demonstrate Sarugaku’s dual expertise: designing cutting-edge observational tools and applying them to unravel the universe’s most violent explosions. With a career defined by technical ingenuity and deep astrophysical insight, Sarugaku remains a vital figure in advancing our understanding of cosmic transients and the instrumentation that captures them.